This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 10.85 18:15:40.49 +13:22:12.2
41.03623 13.88706 galactic Oph Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4497049840907836416 | 18:15:40.40 +13:22:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.691+/-0.028 (K)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 18:15:40.49 +13:22:12.2: 11.77 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 18:15:40.49 +13:22:12.2: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4497049840907836416,2461186.6824,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4497049840907836416 20260526.1824 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 11.26 19:08:49.87 +15:05:43.9
48.33096 3.07261 galactic Aql Second-epoch detections are separated by 2.4" and 6.3 pix
The object was found in VSX18" Gaia DR3 4512662596836316032
Type: SR|M
# Max. Min./Amp. JD0 Period
15.190 G 15.500 G 486.500000000000 M
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:08:49.87 +15:05:43.9: 12.23 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:08:49.87 +15:05:43.9: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4512662596836316032,2461186.6824,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4512662596836316032 20260526.1824 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 11.18 19:10:21.31 +14:11:15.5
47.69325 2.32805 galactic Aql Second-epoch detections are separated by 1.0" and 6.5 pix
The object was found in VSX 2" 2MASS J19102144+1411158
Type: SR
# Max. Min./Amp. JD0 Period
16.132 g Y 0.905 g 2458652.49760 546.274818000000 C
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:10:21.31 +14:11:15.5: 12.26 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:10:21.31 +14:11:15.5: 12.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J19102144+1411158,2461186.6824,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J19102144+1411158 20260526.1824 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 11.27 19:11:36.21 +15:44:09.5
49.20796 2.77351 galactic Aql Second-epoch detections are separated by 1.6" and 6.5 pix
The object was found in VSX 6" Gaia DR3 4512803540487374080
Type: L
# Max. Min./Amp. JD0 Period
14.890 G 15.090 G M
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:11:36.21 +15:44:09.5: 12.20 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:11:36.21 +15:44:09.5: 12.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4512803540487374080,2461186.6824,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4512803540487374080 20260526.1824 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 11.13 19:07:34.03 +14:18:10.6
47.48525 2.98113 galactic Aql Second-epoch detections are separated by 2.1" and 7.0 pix
The object was found in VSX24" ZTF J190732.45+141803.3
Type: EW
# Max. Min./Amp. JD0 Period
18.068 r Y 0.149 r 2458323.75630 0.336812200000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:07:34.03 +14:18:10.6: 12.10 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:07:34.03 +14:18:10.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190732.45+141803.3,2461186.6824,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190732.45+141803.3 20260526.1824 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 11.19 18:57:14.95 +11:52:04.5
44.16769 4.11128 galactic Aql Second-epoch detections are separated by 2.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J284.3106+11.8748 | 18:57:14.94 +11:52:04.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.170+/-0.033 (F)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 18:57:14.95 +11:52:04.5: 12.07 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 18:57:14.95 +11:52:04.5: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J284.3106+11.8748,2461186.6824,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J284.3106+11.8748 20260526.1824 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 11.07 18:52:32.38 +09:53:35.9
41.87770 4.25121 galactic Aql Second-epoch detections are separated by 4.6" and 6.9 pix
The object was found in VSX 6" Gaia DR3 4311339681318551808
Type: RS
# Max. Min./Amp. JD0 Period
12.720 G 12.780 G K
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 18:52:32.38 +09:53:35.9: 12.00 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 18:52:32.38 +09:53:35.9: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4311339681318551808,2461186.6824,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4311339681318551808 20260526.1824 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 10.79 18:16:10.81 +13:30:26.8
41.21804 13.83401 galactic Oph Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4497426522415810048 | 18:16:10.81 +13:30:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.017+/-0.041 (M)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 18:16:10.81 +13:30:26.8: 11.68 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 18:16:10.81 +13:30:26.8: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4497426522415810048,2461186.6824,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4497426522415810048 20260526.1824 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 11.23 19:09:49.90 +14:46:21.7
48.15487 2.70971 galactic Aql Second-epoch detections are separated by 0.8" and 6.7 pix
The object was found in VSX24" Gaia DR3 4320485900082300416
Type:
# Max. Min./Amp. JD0 Period
19.600 G 20.130 G 0.353718000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:09:49.90 +14:46:21.7: 12.21 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:09:49.90 +14:46:21.7: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4320485900082300416,2461186.6824,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4320485900082300416 20260526.1824 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1824 2461186.6824 11.30 19:03:41.98 +13:22:34.7
46.23022 3.39318 galactic Aql Second-epoch detections are separated by 0.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J285.9372+13.3805 | 19:03:41.99 +13:22:34.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.364+/-0.028 (G)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:03:41.98 +13:22:34.7: 12.25 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:03:41.98 +13:22:34.7: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.9372+13.3805,2461186.6824,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J285.9372+13.3805 20260526.1824 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.98982057 27.02.2026 11:45:10.497 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
First image: 2461098.98982057 27.02.2026 11:45:10.497 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Last image: 2461186.68267671 26.05.2026 04:22:53.268 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.98
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 22350
Objects passed selection criteria: 22163
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 12410.5
Average stars matched: 11705.2 (94.3173 %)
Memory usage VmPeak: 126792 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 23:24:51 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.98982057 27.02.2026 11:45:10.497 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
First image: 2461098.98982057 27.02.2026 11:45:10.497 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Last image: 2461186.68267671 26.05.2026 04:22:53.268 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 80
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 27 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 200172
Objects passed selection criteria: 199386
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 117003
Average stars matched: 109915 (93.942 %)
Memory usage VmPeak: 2016380 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 23:32:45 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
SExtractor catalog cache: saved Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat to cache
SExtractor catalog cache: saved Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461186.68219777
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits exists and is non-empty
Saving wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits to local_wcs_cache/
'wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits' -> 'local_wcs_cache/wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits'
wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits exists and is non-empty
Saving wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits to local_wcs_cache/
'wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits' -> 'local_wcs_cache/wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits'
wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits exists and is non-empty
Saving wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits to local_wcs_cache/
'wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits' -> 'local_wcs_cache/wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits'
wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits exists and is non-empty
Saving wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits to local_wcs_cache/
'wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits' -> 'local_wcs_cache/wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits (1st reference image)
verification OK: wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Image size: 937.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:40:01.859 +13:59:41.39 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits (1st new image)
verification OK: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
Image size: 942.6'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:56.422 +13:59:55.67 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:01.859 +13:59:41.39
Second-epoch image center 18:39:56.422 +13:59:55.67
Angular distance between the image centers 0.0223 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits (2nd new image)
verification OK: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Image size: 942.6'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:59.050 +13:59:44.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:40:01.859 +13:59:41.39
Second-epoch image center 18:39:59.050 +13:59:44.45
Angular distance between the image centers 0.0114 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:39:56.422 +13:59:55.67
Second-epoch second image center 18:39:59.050 +13:59:44.45
Angular distance between the image centers 0.01107 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits &> /tmp/tmp.dfQPb3NP8X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits &> /tmp/tmp.QC7TALAqfk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits &> /tmp/tmp.Hh7wOlikHj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits &> /tmp/tmp.Ain6gn0DHQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits and wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits and wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
Found non-empty wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits and wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
The reference image (wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits) and catalog (wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat) found
'wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat' -> 'wcsmag.cat'
Read 23334 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.8228 to 288.3316 deg, Dec +8.5590 to +19.2750 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 271.8228 to 288.3316 deg, Dec 8.5590 to 19.2750 deg
Loaded 15361 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 11425 out of 12454 total matches.
Matched with Tycho-2 12454 out of 23334 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.901300
a=0.000000 b=1.000000 c=22.901300
From vast_summary.log: estimated ref. image limiting mag.: -7.98
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23334 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.8228 to 288.3316 deg, Dec +8.5590 to +19.2750 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 271.8228 to 288.3316 deg, Dec 8.5590 to 19.2750 deg
Loaded 15361 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 11425 out of 12454 total matches.
Matched with Tycho-2 12454 out of 23334 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits:
Forced-photometry filter: calibrated wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits -> calib.txt_param_ref_wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits (aperture=6.4)
Read 25280 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.8177 to 288.3256 deg, Dec +8.5844 to +19.2787 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 271.8177 to 288.3256 deg, Dec 8.5844 to 19.2787 deg
Loaded 15329 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10889 out of 11895 total matches.
Matched with Tycho-2 11895 out of 25280 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits:
Forced-photometry filter: calibrated wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits -> calib.txt_param_ref_wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
2.4 pix Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
2.2 pix fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
2.2 pix fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
2.4 pix wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
2.4 pix wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
Limiting magnitude estimates:
14.9 mag. Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
15.0 mag. Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
11.2 mag. fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
11.1 mag. fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
All-image limiting magnitude estimate: 11.1 (SNR ) 8.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dfQPb3NP8X (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits' -> 'wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
WCS-calibrated image found: wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Checking if the catalog wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat corresponding to the image wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat corresponding to the image wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
WCS catalog name: wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2212, passed=23334
Got 23334 stars (including 21105 good ones) from the SExtractor catalog wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
util/solve_plate_with_UCAC5 got 23334 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 22969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits N_match=964 sigma_overall_arcsec=0.680 sigma_q1_arcsec=0.485 sigma_q2_arcsec=0.972 sigma_q3_arcsec=0.650 sigma_q4_arcsec=0.629 n_q1=231 n_q2=303 n_q3=219 n_q4=211 worst_quadrant_to_overall_ratio=1.430
The image catalog is written to wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits -region wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QC7TALAqfk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits' -> 'wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
WCS_IMAGE_NAME=wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
WCS-calibrated image found: wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
Checking if the catalog wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat corresponding to the image wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat corresponding to the image wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
WCS catalog name: wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2358, passed=25280
Got 25280 stars (including 22900 good ones) from the SExtractor catalog wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat
util/solve_plate_with_UCAC5 got 25280 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits N_match=960 sigma_overall_arcsec=0.627 sigma_q1_arcsec=0.465 sigma_q2_arcsec=0.762 sigma_q3_arcsec=0.583 sigma_q4_arcsec=0.691 n_q1=238 n_q2=298 n_q3=214 n_q4=210 worst_quadrant_to_overall_ratio=1.215
The image catalog is written to wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits -region wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Hh7wOlikHj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
WCS-calibrated image found: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
Checking if the catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat corresponding to the image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat corresponding to the image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
WCS catalog name: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=38, passed=658
Got 658 stars (including 619 good ones) from the SExtractor catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat
util/solve_plate_with_UCAC5 got 658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010473 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 587 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 584 matched stars entering correct_measured_positions(), 515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 584 matched stars entering correct_measured_positions(), 577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 587 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 583 matched stars entering correct_measured_positions(), 585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 583 matched stars entering correct_measured_positions(), 585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 583 stars left (next iteration limit 642)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits N_match=583 sigma_overall_arcsec=0.449 sigma_q1_arcsec=0.545 sigma_q2_arcsec=0.515 sigma_q3_arcsec=0.417 sigma_q4_arcsec=0.369 n_q1=102 n_q2=168 n_q3=160 n_q4=153 worst_quadrant_to_overall_ratio=1.215
The image catalog is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits -region wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Ain6gn0DHQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
WCS-calibrated image found: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Checking if the catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat corresponding to the image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat corresponding to the image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
WCS catalog name: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=40, passed=695
Got 695 stars (including 654 good ones) from the SExtractor catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat
util/solve_plate_with_UCAC5 got 695 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010473 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 627 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 623 matched stars entering correct_measured_positions(), 568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 623 matched stars entering correct_measured_positions(), 628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 627 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 623 matched stars entering correct_measured_positions(), 629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 623 matched stars entering correct_measured_positions(), 629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 623 stars left (next iteration limit 685)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits N_match=623 sigma_overall_arcsec=0.510 sigma_q1_arcsec=0.425 sigma_q2_arcsec=0.584 sigma_q3_arcsec=0.503 sigma_q4_arcsec=0.448 n_q1=113 n_q2=174 n_q3=172 n_q4=164 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits -region wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits sigma_overall=0.680 worst_q_ratio=1.430
ref2=Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits sigma_overall=0.627 worst_q_ratio=1.215
new1=fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits sigma_overall=0.449 worst_q_ratio=1.215
new2=fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits sigma_overall=0.510 worst_q_ratio=1.145
reference average sigma_overall=0.6535 worst_q_ratio=1.3225
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288_astrometric_residuals.png (964 matched stars from wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704_astrometric_residuals.png (960 matched stars from wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078_astrometric_residuals.png (583 matched stars from wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079_astrometric_residuals.png (623 matched stars from wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits'
Saving fully-calibrated image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits'
Preparing the HTML report for the field Her-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32792_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 32792_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:11.59 +09:34:49.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32801_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 32801_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:06:41.41 +09:08:52.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32811_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 32811_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:45.44 +09:22:01.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32813_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 32813_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:05:19.59 +08:46:26.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12686_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 12686_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:05:24.29 +13:51:44.6 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Her-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
SExtractor catalog cache: saved Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat to cache
SExtractor catalog cache: saved Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Creating symlink local_wcs_cache/wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
Creating symlink local_wcs_cache/wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
Creating symlink local_wcs_cache/wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits exists and is non-empty
wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits exists and is non-empty
wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits exists and is non-empty
wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits (1st reference image)
verification OK: wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Image size: 937.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:40:01.859 +13:59:41.39 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits (1st new image)
verification OK: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
Image size: 942.6'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:56.422 +13:59:55.67 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:01.859 +13:59:41.39
Second-epoch image center 18:39:56.422 +13:59:55.67
Angular distance between the image centers 0.0223 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits (2nd new image)
verification OK: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Image size: 942.6'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:39:59.050 +13:59:44.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:40:01.859 +13:59:41.39
Second-epoch image center 18:39:59.050 +13:59:44.45
Angular distance between the image centers 0.0114 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:39:56.422 +13:59:55.67
Second-epoch second image center 18:39:59.050 +13:59:44.45
Angular distance between the image centers 0.01107 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits &> /tmp/tmp.fFsJtA1XYt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits &> /tmp/tmp.qzEO1hJqCd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits &> /tmp/tmp.53ZDZYsCT2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits &> /tmp/tmp.fDpEMHWzGr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits and wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits and wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
Found non-empty wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits and wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
The reference image (wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits) and catalog (wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat) found
'wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat' -> 'wcsmag.cat'
Read 218804 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.8228 to 288.3446 deg, Dec +8.5590 to +19.2753 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 271.8228 to 288.3446 deg, Dec 8.5590 to 19.2753 deg
Loaded 15373 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 9091 out of 13179 total matches.
Matched with Tycho-2 13179 out of 218804 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.724600
a=0.000000 b=1.000000 c=22.724600
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.11
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.11
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 218804 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.8228 to 288.3446 deg, Dec +8.5590 to +19.2753 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 271.8228 to 288.3446 deg, Dec 8.5590 to 19.2753 deg
Loaded 15373 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 9091 out of 13179 total matches.
Matched with Tycho-2 13179 out of 218804 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits:
Forced-photometry filter: calibrated wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits -> calib.txt_param_ref_wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits (aperture=4.7)
Read 228825 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7998 to 288.3256 deg, Dec +8.5824 to +19.2804 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 271.7998 to 288.3256 deg, Dec 8.5824 to 19.2804 deg
Loaded 15357 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8364 out of 12414 total matches.
Matched with Tycho-2 12414 out of 228825 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits:
Forced-photometry filter: calibrated wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits -> calib.txt_param_ref_wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
2.2 pix Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
2.0 pix fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
1.9 pix fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
2.1 pix wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
2.2 pix wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
Limiting magnitude estimates:
15.1 mag. Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
15.2 mag. Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
11.6 mag. fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
11.6 mag. fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.fFsJtA1XYt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits' -> 'wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
WCS-calibrated image found: wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
Checking if the catalog wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat corresponding to the image wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat corresponding to the image wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits
WCS catalog name: wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=32316, passed=218753
Got 218753 stars (including 186174 good ones) from the SExtractor catalog wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat
util/solve_plate_with_UCAC5 got 218753 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 214785 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 214786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 214759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 967 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits N_match=967 sigma_overall_arcsec=0.677 sigma_q1_arcsec=0.455 sigma_q2_arcsec=0.797 sigma_q3_arcsec=0.691 sigma_q4_arcsec=0.690 n_q1=240 n_q2=301 n_q3=209 n_q4=217 worst_quadrant_to_overall_ratio=1.178
The image catalog is written to wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits -region wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qzEO1hJqCd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits' -> 'wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
WCS_IMAGE_NAME=wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
WCS-calibrated image found: wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
Checking if the catalog wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat corresponding to the image wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat corresponding to the image wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits
WCS catalog name: wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=56, blended=35408, passed=228769
Got 228769 stars (including 193109 good ones) from the SExtractor catalog wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat
util/solve_plate_with_UCAC5 got 228769 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 224873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 224872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 224869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits N_match=965 sigma_overall_arcsec=0.670 sigma_q1_arcsec=0.514 sigma_q2_arcsec=0.748 sigma_q3_arcsec=0.627 sigma_q4_arcsec=0.682 n_q1=249 n_q2=305 n_q3=199 n_q4=212 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits -region wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.53ZDZYsCT2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
WCS-calibrated image found: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
Checking if the catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat corresponding to the image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat corresponding to the image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
WCS catalog name: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=144, passed=11085
Got 11085 stars (including 10920 good ones) from the SExtractor catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat
util/solve_plate_with_UCAC5 got 11085 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010473 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 10790 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 10791 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 10791 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits N_match=955 sigma_overall_arcsec=0.456 sigma_q1_arcsec=0.437 sigma_q2_arcsec=0.510 sigma_q3_arcsec=0.445 sigma_q4_arcsec=0.435 n_q1=191 n_q2=280 n_q3=240 n_q4=244 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits -region wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fDpEMHWzGr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
WCS-calibrated image found: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Checking if the catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat corresponding to the image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat corresponding to the image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
WCS catalog name: wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=156, passed=11394
Got 11394 stars (including 11219 good ones) from the SExtractor catalog wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat
util/solve_plate_with_UCAC5 got 11394 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010473 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 11035 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 11038 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 11038 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits N_match=957 sigma_overall_arcsec=0.498 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.550 sigma_q3_arcsec=0.472 sigma_q4_arcsec=0.482 n_q1=201 n_q2=272 n_q3=247 n_q4=237 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits -region wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-11_20.00sec_0.00C_LIGHTs_0078.fits
Saving fully-calibrated image wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Her-10-Q1b1x1_232329_TTUQ1b1x1_1437112_c3lbAxdv/wcs_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079.fits
Preparing the HTML report for the field Her-10-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:07:48.18 +13:09:40.2: 10.97 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:11:20.31 +13:07:05.4: 9.78 +/- 0.00 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:12:58.75 +17:07:50.1: 99.00 +/- 99.00 edge
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:02:08.18 +08:45:32.2: 9.17 +/- 0.00 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:02:52.90 +08:39:21.2: 9.76 +/- 0.00 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:11:20.31 +13:07:05.4: 9.78 +/- 0.00 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:07:48.18 +13:09:40.2: 10.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.78 +/- 0.00
Forced photometry filter REJECTED candidate at 19:11:20.31 +13:07:05.4: ref_mag=9.78 +/- 0.00 new_mean_mag=9.8902 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:02:08.18 +08:45:32.2: 9.14 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 19:07:48.18 +13:09:40.2: ref_mag=10.97 +/- 0.00 new_mean_mag=10.5878 delta=0.38 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:12:58.75 +17:07:50.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 19:12:58.75 +17:07:50.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 9.16 +/- 0.00
Forced photometry filter REJECTED candidate at 19:02:08.18 +08:45:32.2: ref_mag=9.16 +/- 0.00 new_mean_mag=9.6634 delta=-0.51 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:04:18.17 +08:38:57.7: 11.03 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:02:52.90 +08:39:21.2: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 19:02:52.90 +08:39:21.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:06:45.35 +13:32:37.5: 11.27 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:04:18.17 +08:38:57.7: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 19:04:18.17 +08:38:57.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:06:45.35 +13:32:37.5: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.00
Forced photometry filter REJECTED candidate at 19:06:45.35 +13:32:37.5: ref_mag=11.26 +/- 0.00 new_mean_mag=10.9414 delta=0.32 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:04:46.65 +08:37:42.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:02:45.83 +08:46:57.9: 11.05 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:04:46.65 +08:37:42.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 19:04:46.65 +08:37:42.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:02:45.83 +08:46:57.9: 11.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Forced photometry filter REJECTED candidate at 19:02:45.83 +08:46:57.9: ref_mag=11.06 +/- 0.00 new_mean_mag=11.1644 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 18:15:40.49 +13:22:12.2: 11.77 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:08:01.62 +14:41:45.7: 12.31 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:08:49.87 +15:05:43.9: 12.23 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:10:21.31 +14:11:15.5: 12.26 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:11:36.21 +15:44:09.5: 12.20 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:07:34.03 +14:18:10.6: 12.10 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:08:49.87 +15:05:43.9: 12.18 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:08:01.62 +14:41:45.7: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:10:21.31 +14:11:15.5: 12.19 +/- 0.02 detection
Forced photometry filter KEPT candidate at 19:08:49.87 +15:05:43.9: ref_mag=12.20 +/- 0.01 new_mean_mag=11.2516 delta=0.95 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:08:01.62 +14:41:45.7: ref_mag=12.08 +/- 0.01 new_mean_mag=11.1980 delta=0.88 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 18:15:40.49 +13:22:12.2: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter KEPT candidate at 19:10:21.31 +14:11:15.5: ref_mag=12.22 +/- 0.01 new_mean_mag=11.1373 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter KEPT candidate at 18:15:40.49 +13:22:12.2: ref_mag=11.79 +/- 0.01 new_mean_mag=10.7943 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:11:36.21 +15:44:09.5: 12.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 18:57:14.95 +11:52:04.5: 12.07 +/- 0.01 detection
Forced photometry filter KEPT candidate at 19:11:36.21 +15:44:09.5: ref_mag=12.18 +/- 0.01 new_mean_mag=11.2441 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:07:34.03 +14:18:10.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter KEPT candidate at 19:07:34.03 +14:18:10.6: ref_mag=12.07 +/- 0.01 new_mean_mag=11.1306 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 18:57:14.95 +11:52:04.5: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 18:52:32.38 +09:53:35.9: 12.00 +/- 0.01 detection
Forced photometry filter KEPT candidate at 18:57:14.95 +11:52:04.5: ref_mag=12.07 +/- 0.01 new_mean_mag=11.1513 delta=0.92 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 18:52:32.38 +09:53:35.9: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 18:52:32.38 +09:53:35.9: ref_mag=12.00 +/- 0.01 new_mean_mag=11.0724 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 18:16:10.81 +13:30:26.8: 11.68 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:09:49.90 +14:46:21.7: 12.21 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 18:16:10.81 +13:30:26.8: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Forced photometry filter KEPT candidate at 18:16:10.81 +13:30:26.8: ref_mag=11.70 +/- 0.01 new_mean_mag=10.7520 delta=0.94 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:09:49.90 +14:46:21.7: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter KEPT candidate at 19:09:49.90 +14:46:21.7: ref_mag=12.20 +/- 0.01 new_mean_mag=11.1939 delta=1.00 (need > 0.90)
Forced photometry on wcs_Her-10-Q1b1x1_2026-02-27_05-45-10_20.00sec_-14.90C_LIGHT_0288.fits at 19:03:41.98 +13:22:34.7: 12.25 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q1b1x1_2026-03-26_06-31-11_20.00sec_-15.00C_LIGHT_0704.fits at 19:03:41.98 +13:22:34.7: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter KEPT candidate at 19:03:41.98 +13:22:34.7: ref_mag=12.25 +/- 0.01 new_mean_mag=11.2514 delta=1.00 (need > 0.90)
Adding exclusion_list_local.txt__out104338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out145832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72297.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 256737_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256737_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 256738_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256738_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 256744_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256744_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:11.59 +09:34:49.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 256756_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256756_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:06:41.46 +09:08:53.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 256769_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256769_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:45.45 +09:22:01.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 256772_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256772_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:05:19.59 +08:46:25.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 256773_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256773_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:06:27.90 +09:02:03.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 256780_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256780_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:07:11.96 +09:09:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256797_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256797_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 256798_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256798_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 256827_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256827_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 256833_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256833_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:29:55.83 +09:50:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256845_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256845_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:04:43.03 +09:02:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256848_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256848_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:03.33 +09:32:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256856_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256856_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:07:51.18 +09:28:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256877_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256877_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:09:49.99 +10:02:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256884_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256884_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:16.74 +09:48:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256904_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256904_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:42.06 +09:51:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256913_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256913_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:05:45.60 +09:02:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256923_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256923_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:07:41.94 +09:32:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256924_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256924_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 256931_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256931_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 256935_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256935_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:10:02.67 +10:16:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256941_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256941_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:57:06.24 +12:58:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256949_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256949_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:07:52.46 +09:27:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256960_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256960_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:04.28 +09:08:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256962_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256962_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:06.76 +09:26:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256984_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256984_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:42.08 +09:58:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256986_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256986_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:04:51.05 +08:58:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256993_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 256993_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:28:13.57 +11:13:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257010_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 257010_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:10:17.19 +10:10:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257018_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 257018_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:08:06.77 +09:36:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257021_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 257021_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 257031_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 257031_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 257048_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 257048_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:10:16.28 +09:55:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257059_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 257059_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:07:57.90 +09:26:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137757_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 137757_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
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Considering the candidate 104338_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 104338_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 145832_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 145832_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 127572_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 127572_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 158722_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 158722_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 143095_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 143095_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:43.57 +14:56:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129388_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 129388_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 72297_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 72297_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 60932_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 60932_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:11:04.24 +11:30:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24026_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 24026_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 136881_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 136881_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 19:08:46.67 +14:38:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39892_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 39892_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:47:13.65 +10:33:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192320_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 192320_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 17273_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 17273_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:31:02.62 +09:40:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107207_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 107207_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 139850_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 139850_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 35638_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 35638_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:37:19.05 +10:25:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107837_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
Preparing report for the candidate 107837_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
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Considering the candidate 215574_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 215574_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:47:01.31 +18:10:52.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 147242_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 147242_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
**** FOUND 18:59:37.08 +15:04:02.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 122359_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079
The candidate 122359_fd_Her-10-Q1b1x1_2026-05-25_23-22-53_20.00sec_-0.00C_LIGHTs_0079 did not pass the final checks
